
Astrochemistry dives into the evolution of the molecular universe, from the birth of the simplest molecules to the generation of building blocks for planets and possibly life. The universe holds an incredible evolving circular chemistry, where matter is processed and recycled by the birth, life, and death of stars and planets. An astonishing wealth of molecular species is found in space, encompassing the major functional groups in organic chemistry and important biological ones. The harsh conditions created by radiation, shock waves, cosmic rays, and more offer pathways to chemical evolution not possible on planets. Prebiotic molecules and compounds with characteristics relevant to the origin(s) of life on Earth and/or beyond may find their origin in space. This chapter follows the cyclic journey of interstellar matter, passing through the different astronomical environments and their chemical inventories, highlighting landmarks for astrobiology, and ending with future ventures into this fascinating field.
540, 520
540, 520
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 3 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Top 10% | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
